X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068
Abstract NGC 1068 is a source of luminous emission in the near-infrared lines of molecular hydrogen and [Fe II]. Although these emission lines are commonly attributed to shocks, I show that in NGC 1068 it is quite plausible that they arise in the X-Ray Dissociation Region (XDR) produced by X-ray irr...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Maloney, Philip R. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1997 |
|---|
| Schlagwörter: |
|---|
| Anmerkung: |
© Kluwer Academic Publishers 1997 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 248(1997), 1-2 vom: Feb., Seite 105-112 |
|---|---|
| Übergeordnetes Werk: |
volume:248 ; year:1997 ; number:1-2 ; month:02 ; pages:105-112 |
| Links: |
|---|
| DOI / URN: |
10.1023/A:1000548721801 |
|---|
| Katalog-ID: |
OLC2066210404 |
|---|
| LEADER | 01000caa a22002652 4500 | ||
|---|---|---|---|
| 001 | OLC2066210404 | ||
| 003 | DE-627 | ||
| 005 | 20230502213035.0 | ||
| 007 | tu | ||
| 008 | 200820s1997 xx ||||| 00| ||eng c | ||
| 024 | 7 | |a 10.1023/A:1000548721801 |2 doi | |
| 035 | |a (DE-627)OLC2066210404 | ||
| 035 | |a (DE-He213)A:1000548721801-p | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
| 041 | |a eng | ||
| 082 | 0 | 4 | |a 520 |a 530 |a 620 |q VZ |
| 084 | |a 16,12 |2 ssgn | ||
| 100 | 1 | |a Maloney, Philip R. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068 |
| 264 | 1 | |c 1997 | |
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a ohne Hilfsmittel zu benutzen |b n |2 rdamedia | ||
| 338 | |a Band |b nc |2 rdacarrier | ||
| 500 | |a © Kluwer Academic Publishers 1997 | ||
| 520 | |a Abstract NGC 1068 is a source of luminous emission in the near-infrared lines of molecular hydrogen and [Fe II]. Although these emission lines are commonly attributed to shocks, I show that in NGC 1068 it is quite plausible that they arise in the X-Ray Dissociation Region (XDR) produced by X-ray irradiation of the gas in the disk by the powerful active nucleus. This mechanism naturally produces the observed size scale of the H2 emission. I will also briefly discuss the implications of the observations of the pure rotation lines of H2 with ISO (Lutz, this workshop). | ||
| 650 | 4 | |a Molecular Hydrogen | |
| 650 | 4 | |a Column Density | |
| 650 | 4 | |a Surface Brightness | |
| 650 | 4 | |a High Surface Brightness | |
| 650 | 4 | |a Luminous Emission | |
| 773 | 0 | 8 | |i Enthalten in |t Astrophysics and space science |d Kluwer Academic Publishers, 1968 |g 248(1997), 1-2 vom: Feb., Seite 105-112 |w (DE-627)129062723 |w (DE-600)629-4 |w (DE-576)014393522 |x 0004-640X |7 nnns |
| 773 | 1 | 8 | |g volume:248 |g year:1997 |g number:1-2 |g month:02 |g pages:105-112 |
| 856 | 4 | 1 | |u https://doi.org/10.1023/A:1000548721801 |z lizenzpflichtig |3 Volltext |
| 912 | |a GBV_USEFLAG_A | ||
| 912 | |a SYSFLAG_A | ||
| 912 | |a GBV_OLC | ||
| 912 | |a SSG-OLC-TEC | ||
| 912 | |a SSG-OLC-PHY | ||
| 912 | |a SSG-OLC-AST | ||
| 912 | |a SSG-OPC-AST | ||
| 912 | |a GBV_ILN_11 | ||
| 912 | |a GBV_ILN_22 | ||
| 912 | |a GBV_ILN_31 | ||
| 912 | |a GBV_ILN_40 | ||
| 912 | |a GBV_ILN_47 | ||
| 912 | |a GBV_ILN_70 | ||
| 912 | |a GBV_ILN_2002 | ||
| 912 | |a GBV_ILN_2279 | ||
| 912 | |a GBV_ILN_2286 | ||
| 912 | |a GBV_ILN_4012 | ||
| 912 | |a GBV_ILN_4027 | ||
| 912 | |a GBV_ILN_4046 | ||
| 951 | |a AR | ||
| 952 | |d 248 |j 1997 |e 1-2 |c 02 |h 105-112 | ||
| author_variant |
p r m pr prm |
|---|---|
| matchkey_str |
article:0004640X:1997----::ryxiainfoeuahdoeadeim |
| hierarchy_sort_str |
1997 |
| publishDate |
1997 |
| allfields |
10.1023/A:1000548721801 doi (DE-627)OLC2066210404 (DE-He213)A:1000548721801-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Maloney, Philip R. verfasserin aut X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068 1997 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1997 Abstract NGC 1068 is a source of luminous emission in the near-infrared lines of molecular hydrogen and [Fe II]. Although these emission lines are commonly attributed to shocks, I show that in NGC 1068 it is quite plausible that they arise in the X-Ray Dissociation Region (XDR) produced by X-ray irradiation of the gas in the disk by the powerful active nucleus. This mechanism naturally produces the observed size scale of the H2 emission. I will also briefly discuss the implications of the observations of the pure rotation lines of H2 with ISO (Lutz, this workshop). Molecular Hydrogen Column Density Surface Brightness High Surface Brightness Luminous Emission Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 248(1997), 1-2 vom: Feb., Seite 105-112 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:248 year:1997 number:1-2 month:02 pages:105-112 https://doi.org/10.1023/A:1000548721801 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 248 1997 1-2 02 105-112 |
| spelling |
10.1023/A:1000548721801 doi (DE-627)OLC2066210404 (DE-He213)A:1000548721801-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Maloney, Philip R. verfasserin aut X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068 1997 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1997 Abstract NGC 1068 is a source of luminous emission in the near-infrared lines of molecular hydrogen and [Fe II]. Although these emission lines are commonly attributed to shocks, I show that in NGC 1068 it is quite plausible that they arise in the X-Ray Dissociation Region (XDR) produced by X-ray irradiation of the gas in the disk by the powerful active nucleus. This mechanism naturally produces the observed size scale of the H2 emission. I will also briefly discuss the implications of the observations of the pure rotation lines of H2 with ISO (Lutz, this workshop). Molecular Hydrogen Column Density Surface Brightness High Surface Brightness Luminous Emission Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 248(1997), 1-2 vom: Feb., Seite 105-112 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:248 year:1997 number:1-2 month:02 pages:105-112 https://doi.org/10.1023/A:1000548721801 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 248 1997 1-2 02 105-112 |
| allfields_unstemmed |
10.1023/A:1000548721801 doi (DE-627)OLC2066210404 (DE-He213)A:1000548721801-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Maloney, Philip R. verfasserin aut X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068 1997 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1997 Abstract NGC 1068 is a source of luminous emission in the near-infrared lines of molecular hydrogen and [Fe II]. Although these emission lines are commonly attributed to shocks, I show that in NGC 1068 it is quite plausible that they arise in the X-Ray Dissociation Region (XDR) produced by X-ray irradiation of the gas in the disk by the powerful active nucleus. This mechanism naturally produces the observed size scale of the H2 emission. I will also briefly discuss the implications of the observations of the pure rotation lines of H2 with ISO (Lutz, this workshop). Molecular Hydrogen Column Density Surface Brightness High Surface Brightness Luminous Emission Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 248(1997), 1-2 vom: Feb., Seite 105-112 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:248 year:1997 number:1-2 month:02 pages:105-112 https://doi.org/10.1023/A:1000548721801 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 248 1997 1-2 02 105-112 |
| allfieldsGer |
10.1023/A:1000548721801 doi (DE-627)OLC2066210404 (DE-He213)A:1000548721801-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Maloney, Philip R. verfasserin aut X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068 1997 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1997 Abstract NGC 1068 is a source of luminous emission in the near-infrared lines of molecular hydrogen and [Fe II]. Although these emission lines are commonly attributed to shocks, I show that in NGC 1068 it is quite plausible that they arise in the X-Ray Dissociation Region (XDR) produced by X-ray irradiation of the gas in the disk by the powerful active nucleus. This mechanism naturally produces the observed size scale of the H2 emission. I will also briefly discuss the implications of the observations of the pure rotation lines of H2 with ISO (Lutz, this workshop). Molecular Hydrogen Column Density Surface Brightness High Surface Brightness Luminous Emission Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 248(1997), 1-2 vom: Feb., Seite 105-112 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:248 year:1997 number:1-2 month:02 pages:105-112 https://doi.org/10.1023/A:1000548721801 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 248 1997 1-2 02 105-112 |
| allfieldsSound |
10.1023/A:1000548721801 doi (DE-627)OLC2066210404 (DE-He213)A:1000548721801-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Maloney, Philip R. verfasserin aut X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068 1997 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1997 Abstract NGC 1068 is a source of luminous emission in the near-infrared lines of molecular hydrogen and [Fe II]. Although these emission lines are commonly attributed to shocks, I show that in NGC 1068 it is quite plausible that they arise in the X-Ray Dissociation Region (XDR) produced by X-ray irradiation of the gas in the disk by the powerful active nucleus. This mechanism naturally produces the observed size scale of the H2 emission. I will also briefly discuss the implications of the observations of the pure rotation lines of H2 with ISO (Lutz, this workshop). Molecular Hydrogen Column Density Surface Brightness High Surface Brightness Luminous Emission Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 248(1997), 1-2 vom: Feb., Seite 105-112 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:248 year:1997 number:1-2 month:02 pages:105-112 https://doi.org/10.1023/A:1000548721801 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 248 1997 1-2 02 105-112 |
| language |
English |
| source |
Enthalten in Astrophysics and space science 248(1997), 1-2 vom: Feb., Seite 105-112 volume:248 year:1997 number:1-2 month:02 pages:105-112 |
| sourceStr |
Enthalten in Astrophysics and space science 248(1997), 1-2 vom: Feb., Seite 105-112 volume:248 year:1997 number:1-2 month:02 pages:105-112 |
| format_phy_str_mv |
Article |
| institution |
findex.gbv.de |
| topic_facet |
Molecular Hydrogen Column Density Surface Brightness High Surface Brightness Luminous Emission |
| dewey-raw |
520 |
| isfreeaccess_bool |
false |
| container_title |
Astrophysics and space science |
| authorswithroles_txt_mv |
Maloney, Philip R. @@aut@@ |
| publishDateDaySort_date |
1997-02-01T00:00:00Z |
| hierarchy_top_id |
129062723 |
| dewey-sort |
3520 |
| id |
OLC2066210404 |
| language_de |
englisch |
| fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2066210404</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502213035.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s1997 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1023/A:1000548721801</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066210404</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)A:1000548721801-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="a">530</subfield><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Maloney, Philip R.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1997</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Kluwer Academic Publishers 1997</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract NGC 1068 is a source of luminous emission in the near-infrared lines of molecular hydrogen and [Fe II]. Although these emission lines are commonly attributed to shocks, I show that in NGC 1068 it is quite plausible that they arise in the X-Ray Dissociation Region (XDR) produced by X-ray irradiation of the gas in the disk by the powerful active nucleus. This mechanism naturally produces the observed size scale of the H2 emission. I will also briefly discuss the implications of the observations of the pure rotation lines of H2 with ISO (Lutz, this workshop).</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Molecular Hydrogen</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Column Density</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Surface Brightness</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">High Surface Brightness</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Luminous Emission</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Astrophysics and space science</subfield><subfield code="d">Kluwer Academic Publishers, 1968</subfield><subfield code="g">248(1997), 1-2 vom: Feb., Seite 105-112</subfield><subfield code="w">(DE-627)129062723</subfield><subfield code="w">(DE-600)629-4</subfield><subfield code="w">(DE-576)014393522</subfield><subfield code="x">0004-640X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:248</subfield><subfield code="g">year:1997</subfield><subfield code="g">number:1-2</subfield><subfield code="g">month:02</subfield><subfield code="g">pages:105-112</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1023/A:1000548721801</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_31</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2002</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2286</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4027</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">248</subfield><subfield code="j">1997</subfield><subfield code="e">1-2</subfield><subfield code="c">02</subfield><subfield code="h">105-112</subfield></datafield></record></collection>
|
| author |
Maloney, Philip R. |
| spellingShingle |
Maloney, Philip R. ddc 520 ssgn 16,12 misc Molecular Hydrogen misc Column Density misc Surface Brightness misc High Surface Brightness misc Luminous Emission X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068 |
| authorStr |
Maloney, Philip R. |
| ppnlink_with_tag_str_mv |
@@773@@(DE-627)129062723 |
| format |
Article |
| dewey-ones |
520 - Astronomy & allied sciences 530 - Physics 620 - Engineering & allied operations |
| delete_txt_mv |
keep |
| author_role |
aut |
| collection |
OLC |
| remote_str |
false |
| illustrated |
Not Illustrated |
| issn |
0004-640X |
| topic_title |
520 530 620 VZ 16,12 ssgn X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068 Molecular Hydrogen Column Density Surface Brightness High Surface Brightness Luminous Emission |
| topic |
ddc 520 ssgn 16,12 misc Molecular Hydrogen misc Column Density misc Surface Brightness misc High Surface Brightness misc Luminous Emission |
| topic_unstemmed |
ddc 520 ssgn 16,12 misc Molecular Hydrogen misc Column Density misc Surface Brightness misc High Surface Brightness misc Luminous Emission |
| topic_browse |
ddc 520 ssgn 16,12 misc Molecular Hydrogen misc Column Density misc Surface Brightness misc High Surface Brightness misc Luminous Emission |
| format_facet |
Aufsätze Gedruckte Aufsätze |
| format_main_str_mv |
Text Zeitschrift/Artikel |
| carriertype_str_mv |
nc |
| hierarchy_parent_title |
Astrophysics and space science |
| hierarchy_parent_id |
129062723 |
| dewey-tens |
520 - Astronomy 530 - Physics 620 - Engineering |
| hierarchy_top_title |
Astrophysics and space science |
| isfreeaccess_txt |
false |
| familylinks_str_mv |
(DE-627)129062723 (DE-600)629-4 (DE-576)014393522 |
| title |
X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068 |
| ctrlnum |
(DE-627)OLC2066210404 (DE-He213)A:1000548721801-p |
| title_full |
X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068 |
| author_sort |
Maloney, Philip R. |
| journal |
Astrophysics and space science |
| journalStr |
Astrophysics and space science |
| lang_code |
eng |
| isOA_bool |
false |
| dewey-hundreds |
500 - Science 600 - Technology |
| recordtype |
marc |
| publishDateSort |
1997 |
| contenttype_str_mv |
txt |
| container_start_page |
105 |
| author_browse |
Maloney, Philip R. |
| container_volume |
248 |
| class |
520 530 620 VZ 16,12 ssgn |
| format_se |
Aufsätze |
| author-letter |
Maloney, Philip R. |
| doi_str_mv |
10.1023/A:1000548721801 |
| dewey-full |
520 530 620 |
| title_sort |
x-ray excitation of molecular hydrogen and [fe ii] emission in ngc 1068 |
| title_auth |
X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068 |
| abstract |
Abstract NGC 1068 is a source of luminous emission in the near-infrared lines of molecular hydrogen and [Fe II]. Although these emission lines are commonly attributed to shocks, I show that in NGC 1068 it is quite plausible that they arise in the X-Ray Dissociation Region (XDR) produced by X-ray irradiation of the gas in the disk by the powerful active nucleus. This mechanism naturally produces the observed size scale of the H2 emission. I will also briefly discuss the implications of the observations of the pure rotation lines of H2 with ISO (Lutz, this workshop). © Kluwer Academic Publishers 1997 |
| abstractGer |
Abstract NGC 1068 is a source of luminous emission in the near-infrared lines of molecular hydrogen and [Fe II]. Although these emission lines are commonly attributed to shocks, I show that in NGC 1068 it is quite plausible that they arise in the X-Ray Dissociation Region (XDR) produced by X-ray irradiation of the gas in the disk by the powerful active nucleus. This mechanism naturally produces the observed size scale of the H2 emission. I will also briefly discuss the implications of the observations of the pure rotation lines of H2 with ISO (Lutz, this workshop). © Kluwer Academic Publishers 1997 |
| abstract_unstemmed |
Abstract NGC 1068 is a source of luminous emission in the near-infrared lines of molecular hydrogen and [Fe II]. Although these emission lines are commonly attributed to shocks, I show that in NGC 1068 it is quite plausible that they arise in the X-Ray Dissociation Region (XDR) produced by X-ray irradiation of the gas in the disk by the powerful active nucleus. This mechanism naturally produces the observed size scale of the H2 emission. I will also briefly discuss the implications of the observations of the pure rotation lines of H2 with ISO (Lutz, this workshop). © Kluwer Academic Publishers 1997 |
| collection_details |
GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 |
| container_issue |
1-2 |
| title_short |
X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068 |
| url |
https://doi.org/10.1023/A:1000548721801 |
| remote_bool |
false |
| ppnlink |
129062723 |
| mediatype_str_mv |
n |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| doi_str |
10.1023/A:1000548721801 |
| up_date |
2024-07-04T03:59:27.579Z |
| _version_ |
1803619472591814656 |
| fullrecord_marcxml |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2066210404</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502213035.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s1997 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1023/A:1000548721801</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066210404</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)A:1000548721801-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="a">530</subfield><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Maloney, Philip R.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">X-Ray Excitation of Molecular Hydrogen and [Fe II] Emission in NGC 1068</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1997</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Kluwer Academic Publishers 1997</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract NGC 1068 is a source of luminous emission in the near-infrared lines of molecular hydrogen and [Fe II]. Although these emission lines are commonly attributed to shocks, I show that in NGC 1068 it is quite plausible that they arise in the X-Ray Dissociation Region (XDR) produced by X-ray irradiation of the gas in the disk by the powerful active nucleus. This mechanism naturally produces the observed size scale of the H2 emission. I will also briefly discuss the implications of the observations of the pure rotation lines of H2 with ISO (Lutz, this workshop).</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Molecular Hydrogen</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Column Density</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Surface Brightness</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">High Surface Brightness</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Luminous Emission</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Astrophysics and space science</subfield><subfield code="d">Kluwer Academic Publishers, 1968</subfield><subfield code="g">248(1997), 1-2 vom: Feb., Seite 105-112</subfield><subfield code="w">(DE-627)129062723</subfield><subfield code="w">(DE-600)629-4</subfield><subfield code="w">(DE-576)014393522</subfield><subfield code="x">0004-640X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:248</subfield><subfield code="g">year:1997</subfield><subfield code="g">number:1-2</subfield><subfield code="g">month:02</subfield><subfield code="g">pages:105-112</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1023/A:1000548721801</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_31</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2002</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2286</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4027</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">248</subfield><subfield code="j">1997</subfield><subfield code="e">1-2</subfield><subfield code="c">02</subfield><subfield code="h">105-112</subfield></datafield></record></collection>
|
| score |
7.401636 |